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Let us now assess the spatial scales at which the molecular destruction of enstro-
phy occurs. We again denote by u and the scales of the energy-containing velocity
fluctuations. Let us scale the fluctuating vorticity as ω , the mean vorticity gradient
as ω/ , and the fluctuating vorticity gradient as ω/λ 2 , with the magnitude of the
length scale λ 2 to be determined. Our scaling estimates for the leading terms in
Eq. (7.56) are
ω 2 u
ν ω 2
λ 2
,j u j ω
,
νω ,j ω ,j
=
χ ω
,
so that equating the two yields
ν
u
1 / 2
ω 2 u
ν ω 2
λ 2
R 1 / 2
λ 2 ;
.
(7.58)
t
When the turbulence Reynolds number R t is large it follows from (7.58) that there
is a large scale range between and λ 2 , as in three-dimensional turbulence.
As with the Taylor microscale and viscous dissipation in three-dimensional tur-
bulence, we must be cautious in interpreting λ 2 as the spatial scale of the eddies in
which the molecular destruction of enstrophy occurs. Rather, ω/λ 2 is an estimate
of the vorticity gradients. Since the rms vorticity in the dissipative eddies is less
than ω , their length scale is less than λ 2 .
7.5.3 Inertial-range cascades and scaling
Equation (7.58) implies that large- R t two-dimensional turbulence has a large range
of eddy scales r such that
λ 2 . These eddies contain little enstrophy and
do little molecular destruction of it. Interpreted for enstrophy in this inertial range
in two-dimensional turbulence, the scalar variance budget, Eq. (7.4) , indicates that
the enstrophy cascade rate is independent of wavenumber and numerically equal
to χ ω , the mean rate of molecular destruction of enstrophy. If (κ) is the vorticity
spectrum,
r
(κ)dκ = ω 2 ,
(7.59)
0
then the Kolmogorov ( 1941 ) ideas imply that in this inertial subrange
χ 2 / ω κ 1 ,
=
(κ,χ ω )
(7.60)
as pointed out by Kraichnan ( 1967 )and Batchelor ( 1969 ). Since the vorticity spec-
trum is κ 2 times the energy spectrum E(κ) , it follows that the inertial-range energy
spectrum is
E(κ) χ 2 / ω κ 3 .
(7.61)
 
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